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Holmes, J. A.; Lewis, S. R.; Patel, M. R. and Lefèvre, F.
(2018).
URL: https://www.cosmos.esa.int/documents/1499429/15838...
Abstract
To further our understanding of important photochemical processes in the Martian atmosphere, a synthesis can be used to investigate the temporal and spatial agreement between model and observations and determine any possible causes of identified differences. In this study [1], we have assimilated, for the first time, total ozone into a Mars Global Circulation model (GCM) to study the ozone cycle.